
 Data from: 

        "High Resolution Study of Presupernova Compactness"

        by 

        Sukhbold, T., Woosley, S., and Heger, A. 
        (2018, accepted to ApJ on May). 

- Detailed descriptions of calculations are provided in the paper, but 
  please feel free to get in touch with any of us with questions, or 
  if you need something that is not provided here

Contacts:
    Tuguldur  Sukhbold = tuguldur[dot]s[at]gmail[dot]com
    Stan      Woosley  = woosley[at]ucolick[dot]org
    Alexander Heger    = alexander[dot]heger[at]monash[dot]edu
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Following are just brief practical descriptions, for more details please 
see the paper: [arXiv.xxxx.xxxxx]

mdotone.tar.gz
(1.6GB)
- these are ascii tables for 1499 presupernova progenitors with initial 
  masses between 12.00 and 26.99 Msun, from the set with standard mass loss 
  rate (labelled as \dot{M}_N). The filename of each table indicates the 
  initial mass of the model, and they lists final structure and composition 
  quantities for each zone. The column titles are listed at the beginning 
  of files.

mdothalf_*.tar.gz
(4.1GB in total)
- same as mdotone.tar.gz, but for 2799 models with initial masses between 
  12.00 and 39.99 Msun, from the set with half the standard mass loss rate 
  (labelled as \dot{M}_N/2). Due to filesize limits at Harvard-Dataverse, 
  the tables are bundled in 3 pieces.

mdotenth.tar.gz
(99MB)
- same as above, but for 49 models between 12 and 60 Msun from the set with 
  ten times weaker mass loss rate (labelled as \dot{M}_N/10).

convection_plots.tar.gz
(104MB)
- these are 800 convection history plots for models with initial masses between 
  12.00 and 19.99 Msun that had standard mass loss rate (labelled as \dot{M}_N). 
  The format of the figures are identical to those presented in Fig. 12.

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